Model SEDs of Stars from M. Cohen et al.
Calibrated spectral templates assembled from
ground-based and KAO observations from Martin Cohen et al. The individual
files contain information on the
original data (both spectroscopic and photometric). Details about the
overall calibration program can be found in the references listed
here.
- Stars used for the calibration of the Spectral Response Function of
CAM-CVF
- HR 7469
(= HD 185395 = SAO 31815 = HIC 96441), F4V,
(plot)
- HR 7469
(= HD 185395 = SAO 31815 = HIC 96441), F4V,
(plot)
- HR 7310
(= Delta Dra = HD 180711 = SAO 18222 = HIC 94376), G9III,
(plot)
- HR 6705
(= Gamma Dra = HD 164058 = SAO 30653 = HIC 87833), K5III,
(plot)
Model SEDs of stars from P. Hammersley
Calibrated spectral templates provided by Peter Hammersley. Wavelength
coverage is 1-160 microns. The visible
magnitudes and near-infrared photometry observed in the GBPP have
been fitted with a Kurucz model to provide the flux densities at longer
wavelengths. The overall spectral energy distribution is believed to be correct
within 5% . See explanatory
note for more details.
- Stars used for the calibration of the Spectral Response Function of
CAM-CVF
- HR 7341 (= HD 181597 = SAO 48315 = HIC 94890), K1III, (plot
)
Last update: 14-07-2000 by
Pedro Garcia-Lario